A Semi-Implicit, Three-Dimensional Model for Estuarine ... - USGS
A Semi-Implicit, Three-Dimensional Model for Estuarine ... - USGS
A Semi-Implicit, Three-Dimensional Model for Estuarine ... - USGS
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26 A <strong>Semi</strong>-<strong>Implicit</strong>, <strong>Three</strong>-<strong>Dimensional</strong> <strong>Model</strong> <strong>for</strong> <strong>Estuarine</strong> Circulation<br />
and<br />
∂ ∂u<br />
------- ⎛ 1<br />
ν ------- ⎞ ∂ ∂u<br />
------- ⎛ 1<br />
∂x<br />
⎝ t ν ------- ⎞ ∂ ∂u1<br />
+<br />
1 ∂x<br />
⎠<br />
1 ∂x<br />
⎝ t + ------- ⎛ν------- ⎞<br />
2 ∂x<br />
⎠<br />
2 ∂x<br />
⎝ t<br />
3 ∂x<br />
⎠<br />
3<br />
(2.23)<br />
∂ ∂u<br />
------- ⎛ 2<br />
ν ------- ⎞ ∂ ∂u<br />
------- ⎛ 2<br />
∂x<br />
⎝ t<br />
ν ------- ⎞ ∂ ∂u2<br />
+<br />
1 ∂x<br />
⎠<br />
1 ∂x<br />
⎝ t + ------- ⎛ν------- ⎞<br />
2 ∂x<br />
⎠<br />
2 ∂x<br />
⎝ t . (2.24)<br />
3 ∂x<br />
⎠<br />
3<br />
The <strong>for</strong>m of 2.23 and 2.24 does not preserve the symmetry of the turbulent stress tensor because the right sides of<br />
– u1 ′ u′ 2 = νt( ∂u1 ⁄ ∂x2)<br />
and – u2 ′ u′ 1 = νt( ∂u2 ⁄ ∂x1)<br />
are no longer equal as they should be. For this reason, the <strong>for</strong>m of<br />
2.20 and 2.21 sometimes is preferred. It turns out, however, that the loss of symmetry in the stress tensor generally is not a serious<br />
concern <strong>for</strong> estuarine modeling.<br />
When 2.20 and 2.21 or 2.23 and 2.24 is introduced into equation 2.15, the problem of turbulence closure is shifted to that of<br />
defining the distribution of the eddy viscosity. Unlike the molecular viscosity, the eddy viscosity is not a fluid property but instead<br />
varies throughout the flow field as a function of the length and velocity scales of the turbulent eddies. Because the largest-scale<br />
eddies are primarily responsible <strong>for</strong> the turbulent transport of momentum and salt, these largest eddies influence most the magni-<br />
tude of v t. The geometry of the estuary determines to a great extent the size of the largest eddies. Because of the striking disparity<br />
between the length scales of the horizontal and vertical dimensions of most estuaries, the intensity and size of the horizontal eddies<br />
are much greater than those of the vertical eddies. The turbulent motions under these conditions are said to be anisotropic (direction<br />
dependent). It is typical to define separate horizontal and vertical eddy viscosities, A H and A V , to account <strong>for</strong> the anisotropy. The<br />
turbulent stress terms in the <strong>for</strong>m of 2.23 and 2.24 then become<br />
and<br />
∂ ∂u<br />
------- ⎛ 1<br />
A ------- ⎞ ∂ ∂u<br />
------- ⎛ 1<br />
∂x<br />
⎝ H<br />
A ------- ⎞ ∂ ∂u1<br />
+<br />
1 ∂x<br />
⎠<br />
1 ∂x<br />
⎝ H + ------- ⎛A------- ⎞<br />
2 ∂x<br />
⎠<br />
2 ∂x<br />
⎝ V<br />
(2.25)<br />
3 ∂x<br />
⎠<br />
3<br />
∂ ∂u<br />
------- ⎛ 2<br />
A -------- ⎞ ∂ ∂u<br />
------- ⎛ 2<br />
∂x ⎝ H<br />
A -------- ⎞ ∂ ∂u2 +<br />
1 ∂x ⎠<br />
1 ∂x ⎝ H + ------- ⎛A-------- ⎞<br />
2 ∂x ⎠<br />
2 ∂x ⎝ V . (2.26)<br />
3 ∂x ⎠<br />
3<br />
For estuaries, a possible range of magnitudes is 10 3 to 10 6 cm 2 /s <strong>for</strong> A H and 1 to 500 cm 2 /s <strong>for</strong> A V.<br />
Because of the large horizontal extent of flow in most estuaries, the horizontal variations in mean-flow quantities generally<br />
are much more gradual than the vertical variations. As a result, the four terms in 2.25 and 2.26 involving horizontal gradients of<br />
mean velocities ordinarily are much smaller than the two terms involving vertical gradients. (This will be demonstrated also in<br />
Section 2.5 using scale analysis.) Each of the terms in 2.25 and 2.26 represent momentum diffusion due to turbulence in addition<br />
to their interpretation as stresses. Horizontal momentum diffusion generally is less significant in estuaries than vertical momentum<br />
diffusion.